Derives the fifth action for 1.5PN BBH with arbitrary eccentricity, spins, and masses, completing action-angle variables for analytical dynamics solution.
Since the flows underJ2,L 2,S 2 1, and S2 2 do not change these mutual angles, we choose to flow under Seff·L by exactly the precession period, ∆λSeff·L = Λ
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Action-angle variables of a binary black hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order
Derives the fifth action for 1.5PN BBH with arbitrary eccentricity, spins, and masses, completing action-angle variables for analytical dynamics solution.